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Solar Neutrinos as Background to Neutrinoless Double-beta Decay Experiments

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arxiv 1708.00927 v1 pith:K7Y6GRSF submitted 2017-08-02 nucl-ex physics.ins-det

classification nucl-exphysics.ins-det
keywords experimentssolarneutrinobackgroundbackgroundsdecaydouble-betafuture
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abstract

Solar neutrinos interact within double-beta decay (\BB) detectors and contribute to backgrounds for \BB\ experiments. Background contributions due to charge-current solar neutrino interactions with \BB\ nuclei of $^{76}$Ge, $^{82}$Se, $^{100}$Mo, $^{130}$Te, $^{136}$Xe, and $^{150}$Nd are evaluated. They are shown to be significant for future high-sensitivity \BB\ experiments that may search for Majorana neutrino masses in the inverted-hierarchy mass region. The impact of solar neutrino backgrounds and their reduction are discussed for future \BB\ experiments.

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Cited by 1 Pith paper

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  1. The lowest-radiation environments in the Solar System: new opportunities for underground rare-event searches

    hep-ex 2024-11 conditional novelty 6.0 of 10

    Atmospherless bodies in the Solar System suppress cosmic-ray-induced neutrino and muon fluxes by about three to four orders of magnitude, opening new sites for ultra-low-background rare-event searches.

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